Physical processes in pulsar magnetospheres and non-thermal high-frequency emission

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dc.creatorUsov, Vladimir V.
dc.date1996-12-09
dc.date.accessioned2026-07-07T02:22:29Z
dc.date.available2026-07-07T02:22:29Z
dc.descriptionThe energy source of a pulsar's non-thermal emission is the rotational energy loss of the neutron star. The rotational energy of the neutron star is transformed into the pulsar radiation by a long sequence of processes. The processes of this sequence are discussed.
dc.description8 pages, latex, no figures. To be published in the Proceedings of the IAU Colloquium No 160, Pulsars: Problems and Progress, Sydney, 8-12 January 1996 (invited paper)
dc.identifierhttps://arxiv.org/abs/astro-ph/9612078
dc.identifierhttp://arxiv.org/abs/astro-ph/9612078
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10895
dc.subjectAstrophysics
dc.titlePhysical processes in pulsar magnetospheres and non-thermal high-frequency emission
dc.typetext

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